Her primary areas of study are Astrophysics, Galaxy, Astronomy, Stellar population and Metallicity. Her Astrophysics research includes elements of Spectral line and Spectral resolution. Galaxy connects with themes related to Starlight in her study.
Her Surface brightness, Galaxy cluster, Disc and Bulge study in the realm of Astronomy connects with subjects such as Christian ministry. As part of one scientific family, Patricia Sanchez-Blazquez deals mainly with the area of Stellar population, narrowing it down to issues related to the Radius, and often Morphological type and Critical value. Her work deals with themes such as Spiral galaxy and Velocity dispersion, which intersect with Metallicity.
Her primary scientific interests are in Astrophysics, Galaxy, Astronomy, Star formation and Stellar population. Metallicity, Elliptical galaxy, Stars, Velocity dispersion and Galaxy formation and evolution are among the areas of Astrophysics where the researcher is concentrating her efforts. Her Stars research integrates issues from Interstellar medium and Supernova.
Galaxy is closely attributed to Spectral line in her work. Her Star formation study combines topics in areas such as Luminosity, Radius and Effective radius. Her Stellar population study deals with Spectral resolution intersecting with Telescope.
Her primary areas of study are Astrophysics, Galaxy, Star formation, Metallicity and Stellar population. Her Astrophysics study frequently draws parallels with other fields, such as Radius. As part of her studies on Galaxy, Patricia Sanchez-Blazquez frequently links adjacent subjects like Stars.
The study incorporates disciplines such as Local Group, Dwarf galaxy, Galaxy formation and evolution and Spatially resolved in addition to Star formation. Her Metallicity research focuses on Line and how it relates to Interstellar medium. Patricia Sanchez-Blazquez has researched Stellar population in several fields, including Extinction, Spectral energy distribution and Universe.
Her main research concerns Astrophysics, Galaxy, Stellar population, Star formation and Metallicity. Astrophysics and Radius are commonly linked in her work. Her work on Secular evolution, Spiral galaxy, Redshift and Luminosity as part of general Galaxy study is frequently connected to Bar, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them.
Stellar population and Universe are frequently intertwined in her study. Her Star formation research focuses on Velocity dispersion and how it connects with Star cluster. The various areas that Patricia Sanchez-Blazquez examines in her Metallicity study include Large Magellanic Cloud and Local Group, Leo A, Dwarf galaxy.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
MILES: A Medium resolution INT Library of Empirical Spectra
Patricia Sanchez-Blazquez;Reynier Peletier;Jorge Jimenez-Vicente;Nicolas Cardiel.
arXiv: Astrophysics (2006)
Medium-resolution isaac newton telescope library of empirical spectra
P. Sanchez-Blazquez;P. Sanchez-Blazquez;P. Sanchez-Blazquez;R. F. Peletier;R. F. Peletier;J. Jimenez-Vicente;N. Cardiel.
Monthly Notices of the Royal Astronomical Society (2006)
CALIFA, the Calar Alto Legacy Integral Field Area survey : I. Survey presentation
S. F. Sánchez;R. C. Kennicutt;A. Gil de Paz;G. van de Ven.
Astronomy and Astrophysics (2012)
Evolutionary stellar population synthesis with MILES: I. The base models and a new line index system
A. Vazdekis;A. Vazdekis;P. Sánchez-Blázquez;P. Sánchez-Blázquez;J. Falcón-Barroso;J. Falcón-Barroso;A. J. Cenarro;A. J. Cenarro.
Monthly Notices of the Royal Astronomical Society (2010)
An updated MILES stellar library and stellar population models (Research Note)
J. Falcon-Barroso;P. Sanchez-Blazquez;A. Vazdekis;E. Ricciardelli.
Astronomy and Astrophysics (2011)
An updated MILES stellar library and stellar population models
J. Falcón-Barroso;P. Sánchez-Blázquez;A. Vazdekis;E. Ricciardelli.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
The O3N2 and N2 abundance indicators revisited: improved calibrations based on CALIFA and Te-based literature data
R. A. Marino;F. F. Rosales-Ortega;S. F. Sánchez;A. Gil de Paz.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
A characteristic oxygen abundance gradient in galaxy disks unveiled with CALIFA
S. F. Sanchez;F. F. Rosales-Ortega;J. Iglesias-Paramo;M. Molla.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
Evolutionary Stellar Population Synthesis with MILES. Part I: The Base Models and a New Line Index System
A. Vazdekis;P. Sánchez-Blázquez;J. Falcón-Barroso;A. J. Cenarro.
arXiv: Cosmology and Nongalactic Astrophysics (2010)
The O3N2 and N2 abundance indicators revisited: improved calibrations based on CALIFA and T e-based literature data
R. A. Marino;F. F. Rosales-Ortega;F. F. Rosales-Ortega;Sebastian Francisco Sanchez Sanchez;A. Gil De Paz.
Astronomy and Astrophysics (2013)
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